Spectral and Spatial Variations of Flare Hard X-ray Footpoints |
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Authors: | Fletcher L Hudson HS |
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Institution: | (1) Department of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, U.K.;(2) Space Sciences Laboratory, University of California, Berkeley, CA, 94720-7450, U.S.A. |
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Abstract: | In a sample of strong RHESSI M-class flares we have made a study of the relationship between the `hardness' of the HXR spectrum
and the intensity in the 30–50 keV energy range. In all events we find clear evidence for a `soft–hard–soft' pattern of correlation
between hardness and flux, on time scales as short as 10 s. We investigate whether or not this pattern is intrinsic to the
acceleration mechanism. The RHESSI images in this energy range are dominated by footpoint brightenings, and we have searched
for a correlation between footpoint separation velocity and spectral hardness, to be compared qualitatively with theoretical
flare models. We find quite systematic footpoint motions, and also note that episodes in which footpoint separation varies
rapidly often correspond with episodes of significant change in the flare spectral index, though not as the simplest flare
models would predict. We report also on one of our events, on 14 March 2002, which exhibits highly sheared HXR footpoint ribbons
extending over a scale of 100 arc sec. For this flare we find a correlation between footpoint motion and hard X-ray flux.
Supplementary material to this paper is available in electronic form at http://dx.doi.org/10.1023/A:1022479610710 |
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